Acceleration due to gravity: Difference between revisions

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In the [[science]]s, the term '''acceleration due to gravity''' commonly refers to the value of 9.80656 m/s<sup>2</sup> and is denoted as ''g<sub>n</sub>''. That value was agreed upon by the 3rd General Conference on Weights and Measures (Conférence Générale des Poids et Mesures, CGPM) in 1901.<ref>[http://physics.nist.gov/Document/sp330.pdf The International System of Units (SI), NIST Special Publication 330, 2001 Edition] (pdf page 29 of 77 pdf pages) </ref><ref>[http://www.bipm.org/utils/common/pdf/si_brochure_8_en.pdf#page=51 Bureau International des Poids et Mesures] (pdf page 51 of 88 pdf pages)</ref> It is also often referred to as the ''local gravitational acceleration'' or the ''standard gravity''.
{{subpages}}
Where ''g'' is the '''acceleration due to gravity''', an object with mass ''m'' near the surface of Earth experiences a downward gravitational force of magnitude ''mg''. The quantity ''g'' has the dimension of acceleration, m s<sup>&minus;2</sup>, hence its name. Equivalently, it can be expressed in terms of force per unit mass, or N/kg in SI units.


Any object near the [[earth]] is subject to a [[force]] in the downward direction that causes an [[acceleration]] of magnitude ''g<sub>n</sub>'' toward the surface of the earth. This value serves as an excellent approximation for the local acceleration due to gravity at the surface of the earth, although it is not exact and the actual acceleration varies slightly between different locations around the world.
[[Gravitation#Newton's law of universal gravitation|Newton's gravitational law]] gives the following formula for ''g'',
:<math>g = G\, \frac{M_{\mathrm{E}}}{R^2_{\mathrm{E}}},</math>
where ''G'' is the universal gravitational constant,<ref> Source: [http://physics.nist.gov/cgi-bin/cuu/Value?bg|search_for=Gravitational  CODATA 2006, retrieved 2/24/08 from NIST website]</ref> ''G'' = 6.67428 &times; 10<sup>&minus;11</sup>
m<sup>3</sup> kg<sup>&minus;1</sup> s<sup>&minus;2</sup>,
''M''<sub>E</sub> is the total mass of Earth, and ''R''<sub>E</sub> is the radius of Earth. This equation gives a good approximation, but is not exact. Deviations are caused by the [[centrifugal force]] due to the rotation of Earth around its axis, non-sphericity of Earth, and the non-homogeneity of the composition of Earth. These effects cause ''g'' to vary roughly &plusmn; 0.02 around the value 9.8 m s<sup>&minus;2</sup> from place to place on the surface of Earth. The quantity ''g'' is therefore referred to as the ''local gravitational acceleration''. It is measured as 9.78 m s<sup>&minus;2</sup> at the equator and 9.83 m s<sup>&minus;2</sup> at the poles.


More generally the acceleration due to gravity refers to the magnitude of some test object due to the [[mass]] of another object. Under [[Newtonian gravity]] the gravitational field strength, due to a [[spherical symmetry|spherically symmetric]] object of mass ''M'' is given by:
The 3rd [[General Conference on Weights and Measures]] (Conférence Générale des Poids et Mesures, CGPM) defined in 1901 a standard value denoted as ''g<sub>n</sub>''.<ref>[http://physics.nist.gov/Document/sp330.pdf The International System of Units (SI), NIST Special Publication 330, 2001 Edition] (pdf page 29 of 77 pdf pages)</ref>
:<math>g = G \frac{M}{r^2} </math>
<ref>[http://www.bipm.org/utils/common/pdf/si_brochure_8_en.pdf Bureau International des Poids et Mesures] (Brochure on SI, pdf page 51 of 88 pdf pages) From the website of the [[Bureau International des Poids et Mesures]]</ref> The value of the ''standard acceleration due to gravity'' ''g<sub>n</sub>'' is 9.80665 m s<sup>&minus;2</sup>. This value of ''g<sub>n</sub>'' was the conventional reference for calculating the now obsolete unit of force, the kilogram force, as the force needed for one kilogram of ''mass'' to accelerate at this value.
The magnitude of the acceleration is in [[SI]] units of [[meter]]s per [[second]] squared.
Here ''G'' is the [[universal gravitational constant]], ''G'' = 6.67428&times;10<sup>&minus;11</sup> Nm<sup>2</sup>/kg<sup>2</sup>,<ref> Source: [http://physics.nist.gov/cgi-bin/cuu/Value?bg|search_for=Gravitational  CODATA 2006, retrieved 2/24/08 from NIST website]</ref> <math>r</math> is the distance of the test object to the centre of mass  of the Earth and ''M'' is the mass of the Earth.  


In physics [[acceleration]] is a vector, with an absolute value (magnitude, length) ''g''  and a direction from the center of mass of Earth toward the test object, hence as a vector the acceleration is,
==References==
:<math>
{{reflist}}
\vec{g} = - G \frac{M}{r^2} \vec{e}_r \quad \hbox{with}\quad \vec{e}_r \equiv \frac{\vec{r}}{r}.
</math>


==Reference==
[[Category:Suggestion Bot Tag]]
<references />
[[Category: CZ Live]]
[[Category: Physics Workgroup]]

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Where g is the acceleration due to gravity, an object with mass m near the surface of Earth experiences a downward gravitational force of magnitude mg. The quantity g has the dimension of acceleration, m s−2, hence its name. Equivalently, it can be expressed in terms of force per unit mass, or N/kg in SI units.

Newton's gravitational law gives the following formula for g,

where G is the universal gravitational constant,[1] G = 6.67428 × 10−11 m3 kg−1 s−2, ME is the total mass of Earth, and RE is the radius of Earth. This equation gives a good approximation, but is not exact. Deviations are caused by the centrifugal force due to the rotation of Earth around its axis, non-sphericity of Earth, and the non-homogeneity of the composition of Earth. These effects cause g to vary roughly ± 0.02 around the value 9.8 m s−2 from place to place on the surface of Earth. The quantity g is therefore referred to as the local gravitational acceleration. It is measured as 9.78 m s−2 at the equator and 9.83 m s−2 at the poles.

The 3rd General Conference on Weights and Measures (Conférence Générale des Poids et Mesures, CGPM) defined in 1901 a standard value denoted as gn.[2] [3] The value of the standard acceleration due to gravity gn is 9.80665 m s−2. This value of gn was the conventional reference for calculating the now obsolete unit of force, the kilogram force, as the force needed for one kilogram of mass to accelerate at this value.

References